Connections Between the Non-Migrating Semidiurnal Tide Over the South Pole and Stationary Planetary Waves in the Northern Hemisphere
The westward propagating zonal wavenumber 1 non-migrating semidiurnal tide is a dominant dynamical feature present during the Austral summer over the South Pole. It has been hypothesized that this wave is generated by a non-linear interaction between the zonal wavenumber one stationary planetary wav...
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ftunicolboulder:oai:scholar.colorado.edu:asen_gradetds-1042 2023-05-15T18:21:51+02:00 Connections Between the Non-Migrating Semidiurnal Tide Over the South Pole and Stationary Planetary Waves in the Northern Hemisphere Estante, Frederico Eduardo da Cunha 2012-01-01T08:00:00Z application/pdf https://scholar.colorado.edu/asen_gradetds/42 https://scholar.colorado.edu/cgi/viewcontent.cgi?article=1042&context=asen_gradetds unknown CU Scholar https://scholar.colorado.edu/asen_gradetds/42 https://scholar.colorado.edu/cgi/viewcontent.cgi?article=1042&context=asen_gradetds Aerospace Engineering Sciences Graduate Theses & Dissertations Atmospheric Tide Planetary Wave semidiurnal non-migrating South Pole stationary planetary wave Aerospace Engineering Atmospheric Sciences text 2012 ftunicolboulder 2018-10-07T08:49:45Z The westward propagating zonal wavenumber 1 non-migrating semidiurnal tide is a dominant dynamical feature present during the Austral summer over the South Pole. It has been hypothesized that this wave is generated by a non-linear interaction between the zonal wavenumber one stationary planetary wave in the northern hemisphere stratosphere and the zonal wavenumber two migrating diurnal tide. However, direct evidence of this interaction has yet to be observed. Using observations from the South Pole meteor radar (SPMR) system we can unam- biguously determine the structure of the non-migrating semidiurnal tide in the meridional wind field. These observations are correlated with the stationary planetary wave activity in the zonal and meridional wind fields in the northern hemisphere stratosphere. Data from the NASA Modern Era Retrospective-Analysis for Research and Applications (MERRA) global assimilative model are used to determine the structure of the zonal wavenumber 1,2, and 3 stationary planetary waves for this comparison. In addition, temperature data from the NASA TIMED SABER mission was analyzed and compared to the MERRA temperature observations as validation of the MERRA model results. Correlation analysis has indicated periods of time with significant correlation be- tween the zonal wave-number 1 stationary planetary wave and the SPMR data and other times with very strong anti-correlations. Similar features are observed with the zonal wave- number 3 stationary planetary wave. Text South pole University of Colorado, Boulder: CU Scholar Austral South Pole Merra ENVELOPE(12.615,12.615,65.816,65.816) |
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Open Polar |
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University of Colorado, Boulder: CU Scholar |
op_collection_id |
ftunicolboulder |
language |
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topic |
Atmospheric Tide Planetary Wave semidiurnal non-migrating South Pole stationary planetary wave Aerospace Engineering Atmospheric Sciences |
spellingShingle |
Atmospheric Tide Planetary Wave semidiurnal non-migrating South Pole stationary planetary wave Aerospace Engineering Atmospheric Sciences Estante, Frederico Eduardo da Cunha Connections Between the Non-Migrating Semidiurnal Tide Over the South Pole and Stationary Planetary Waves in the Northern Hemisphere |
topic_facet |
Atmospheric Tide Planetary Wave semidiurnal non-migrating South Pole stationary planetary wave Aerospace Engineering Atmospheric Sciences |
description |
The westward propagating zonal wavenumber 1 non-migrating semidiurnal tide is a dominant dynamical feature present during the Austral summer over the South Pole. It has been hypothesized that this wave is generated by a non-linear interaction between the zonal wavenumber one stationary planetary wave in the northern hemisphere stratosphere and the zonal wavenumber two migrating diurnal tide. However, direct evidence of this interaction has yet to be observed. Using observations from the South Pole meteor radar (SPMR) system we can unam- biguously determine the structure of the non-migrating semidiurnal tide in the meridional wind field. These observations are correlated with the stationary planetary wave activity in the zonal and meridional wind fields in the northern hemisphere stratosphere. Data from the NASA Modern Era Retrospective-Analysis for Research and Applications (MERRA) global assimilative model are used to determine the structure of the zonal wavenumber 1,2, and 3 stationary planetary waves for this comparison. In addition, temperature data from the NASA TIMED SABER mission was analyzed and compared to the MERRA temperature observations as validation of the MERRA model results. Correlation analysis has indicated periods of time with significant correlation be- tween the zonal wave-number 1 stationary planetary wave and the SPMR data and other times with very strong anti-correlations. Similar features are observed with the zonal wave- number 3 stationary planetary wave. |
format |
Text |
author |
Estante, Frederico Eduardo da Cunha |
author_facet |
Estante, Frederico Eduardo da Cunha |
author_sort |
Estante, Frederico Eduardo da Cunha |
title |
Connections Between the Non-Migrating Semidiurnal Tide Over the South Pole and Stationary Planetary Waves in the Northern Hemisphere |
title_short |
Connections Between the Non-Migrating Semidiurnal Tide Over the South Pole and Stationary Planetary Waves in the Northern Hemisphere |
title_full |
Connections Between the Non-Migrating Semidiurnal Tide Over the South Pole and Stationary Planetary Waves in the Northern Hemisphere |
title_fullStr |
Connections Between the Non-Migrating Semidiurnal Tide Over the South Pole and Stationary Planetary Waves in the Northern Hemisphere |
title_full_unstemmed |
Connections Between the Non-Migrating Semidiurnal Tide Over the South Pole and Stationary Planetary Waves in the Northern Hemisphere |
title_sort |
connections between the non-migrating semidiurnal tide over the south pole and stationary planetary waves in the northern hemisphere |
publisher |
CU Scholar |
publishDate |
2012 |
url |
https://scholar.colorado.edu/asen_gradetds/42 https://scholar.colorado.edu/cgi/viewcontent.cgi?article=1042&context=asen_gradetds |
long_lat |
ENVELOPE(12.615,12.615,65.816,65.816) |
geographic |
Austral South Pole Merra |
geographic_facet |
Austral South Pole Merra |
genre |
South pole |
genre_facet |
South pole |
op_source |
Aerospace Engineering Sciences Graduate Theses & Dissertations |
op_relation |
https://scholar.colorado.edu/asen_gradetds/42 https://scholar.colorado.edu/cgi/viewcontent.cgi?article=1042&context=asen_gradetds |
_version_ |
1766201183620300800 |